Homepage of Stéphane Blondin
Download the Supernova Identification (SNID) code here
I am an astrophysicist at the Laboratoire d'Astrophysique de Marseille
(LAM). My research mainly revolves around the analysis of radiation from exploding
stars known as supernovae.
At LAM I lead the Transients discussion group.
I defended my PhD thesis, entitled
"Optical Spectra of Thermonuclear Supernovae in the
Local and Distant Universe", at the
(Munich, Germany) in November 2005.
During my postdoc at the Harvard-Smithsonian Center for Astrophysics (CfA) I founded the CfA Supernova Archive, where you can freely download light curves and spectra of many supernovae.
You can view my CV here [pdf]
Supernova model results
Repository of the results from our numerical simulations on supernovae:
This research has benefited from funding by the Agence Nationale de la Recherche from 2011 to 2016, under grant number ANR-2011-Blanc-SIMI-5-6-007-01.
See the project description here: RTCCSN.
[more under Publications
Evidence for sub-Chandrasekhar-mass progenitors of Type Ia supernovae at the faint end of the width-luminosity relation [astro-ph
Blondin, S., Dessart, L., Hillier, D. J., Khokhlov, A. M. 2017. Accepted for publication in MNRAS
A one-dimensional Chandrasekhar-mass delayed-detonation model for the broad-lined Type Ia supernova 2002bo
, Dessart, L., Hillier, D. J. 2015. MNRAS, 448, 2766.
The hydrodynamical input and synthetic spectra are available here
One-dimensional delayed-detonation models of Type Ia supernovae: Confrontation to observations at bolometric maximum
, Dessart, L., Hillier, D. J., Khokhlov, A. M. 2013. MNRAS, 429, 2127.
The maximum-light spectra of the DDC model series can be downloaded here
. Also included are the hydro grid (velocity, density) and abundance
profiles for 56
Ni, Ni, Si, and O within 20-60 s from explosion.
Last updated on: 13 Jan 2017